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By identifying the recently introduced Barbero-Immirzi field with the QCD axion, the strong CP problem can be solved through the Peccei-Quinn mechanism.
R.D. Peccei and H.R. Quinn, Phys. Rev. Lett. 38
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E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, New York, 1994); M.Yu. Khlopov, Cosmoparticle Physics (World Scientific, Singapore, 1999)
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The field β \beta is usually referred to as the Barbero-Immirzi (BI) field; see, V. Taveras and N. Yunes, Phys. Rev. D 78
2009
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S. Mercuri and V. Taveras, Phys. Rev. D 80
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The signature throughout the paper is ( + , − , − , − ) (+,-,-,-) with ϵ 0123 = 1 \epsilon_{0123}=1 . For convenience, we set ℏ = c = k B = 1 \hbar=c=k_{B}=1 and 8 π G = k 8\pi G=k
S. Alexander and N. Yunes, Phys. Rept. 480
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N. Yunes and F. Pretorius, Phys. Rev. D 79
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S.J. Gates, S.V. Ketov, and N. Yunes, Phys. Rev. D 80
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E. Komatsu et al
2009
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L. Visinelli and P. Gondolo, Phys. Rev. D 80
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R.D. Peccei, arXiv:hep-ph/9807516
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It is worth remarking that, even postulating the existence of an additional U ( 1 ) P Q U(1)_{PQ} chiral symmetry, the electroweak CP
Cited in the paper.
The imaginary unit i i disappears in Minkowski space
Cited in the paper.
It is worth remarking that the BI field turns out to be a pseudoscalar as suggested by its contribution to the irreducible torsion components [ 11 ] and confirmed by its equations of motion [ 13 ]
Cited in the paper.
Thermal production is excluded by astrophysical constraints
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